activity
19962019
most citedThe Chandra Deep Field South: the 1 Million Second

614 citations · 4k across the 33 of their papers we have counts for

collaborators

33 papers

astro-ph.SR2019★ 56 cited

A UV and optical study of 18 old novae with Gaia DR2 distances: mass accretion rates, physical parameters, and MMRD

Pierluigi Selvelli, Roberto Gilmozzi

{We combine the results of our earlier study of the UV characteristics of 18 classical novae (CNe) with data from the literature and with the recent precise distance determinations…

astro-ph.SR2018★ 8 cited

On the chemical abundances of Miras in clusters: V1 in the metal-rich globular NGC 5927

V. D'Orazi, D. Magurno, G. Bono +50

We present the first spectroscopic abundance determination of iron, alpha-elements (Si, Ca and Ti) and sodium for the Mira variable V1 in the metal-rich globular cluster NGC 5927.…

astro-ph.GA2015★ 36 cited

The Carina Project. VIII. The α-element abundances

M. Fabrizio, M. Nonino, G. Bono +16

We have performed a new abundance analysis of Carina Red Giant (RG) stars from spectroscopic data collected with UVES (high resolution) and FLAMES/GIRAFFE (high and medium resoluti…

astro-ph.IM2014★ 4 cited

On the use of asymmetric PSF on NIR images of crowded stellar fields

Giuliana Fiorentino, Ivan Ferraro, Giacinto Iannicola +8

We present data collected using the camera PISCES coupled with the Firt Light Adaptive Optics (FLAO) mounted at the Large Binocular Telescope (LBT). The images were collected using…

astro-ph.IM2014

Stellar populations in the ELT perspective

G. Bono, V. F. Braga, M. Fabrizio +11

We discuss the impact that the next generation of Extremely Large Telescopes will have on the open astrophysical problems of resolved stellar populations. In particular, we address…

astro-ph.CO2012★ 31 cited

The Carina Project. V. The impact of NLTE effects on the iron content

M. Fabrizio, T. Merle, F. Thévenin +21

We have performed accurate iron abundance measurements for 44 red giants (RGs) in the Carina dwarf spheroidal (dSph) galaxy. We used archival, high-resolution spectra (R~38,000) co…